MOA-2007-BLG-387Lb light curve I band Virtual Observatory Resource

Authors

1. Batista V.
2. Gould A.
3. Dieters S.
4. Dong Subo
5. Bond I.
6. Beaulieu J.P.,Maoz D.
7. Monard B.
8. Christie G.W.
9. McCormick J.
10. Albrow M.D.
11. Horne K.,Tsapras Y.
12. Burgdorf M.J.
13. Calchi Novati S.
14. Skottfelt J.
15. Caldwell J.,Kozlowski S.
16. Kubas D.
17. Gaudi B.S.
18. Han C.
19. Bennett1 D.P.
20. An J.,Abe F.
21. Botzler C.S.
22. Douchin D.
23. Freeman M.
24. Fukui A.
25. Furusawa K.,Hearnshaw J.B.
26. Hosaka S.
27. Itow Y.
28. Kamiya K.
29. Kilmartin P.M.
30. Korpela A.,Lin W.
31. Ling C.H.
32. Makita S.
33. Masuda K.
34. Matsubara Y.
35. Miyake N.,Muraki Y.
36. Nagaya M.
37. Nishimoto K.
38. Ohnishi K.
39. Okumura T.
40. Perrott Y.C.,Rattenbury N.
41. Saito To.
42. Sullivan D.J.
43. Sumi T.
44. Sweatman W.L.,Tristram P.J.
45. von Seggern E.
46. Yock P.C.M. (The MOA Collaboration),Brillant S.
47. Calitz J.J.
48. Cassan A.
49. Cole A.
50. Cook K.
51. Coutures C.,Dominis Prester D.
52. Donatowicz J.
53. Greenhill J.
54. Hoffman M.
55. Jablonski F.,Kane S.R.
56. Kains N.
57. Marquette J.-B.
58. Martin R.
59. Martioli E.
60. Meintjes P.,Menzies J.
61. Pedretti E.
62. Pollard K.
63. Sahu K.C.
64. Vinter C.
65. Wambsganss J.,Watson R.
66. Williams A.
67. Zub M. (The PLANET Collaboration),Allen W.
68. Bolt G.
69. Bos M.
70. DePoy D.L.
71. Drummond J.
72. Eastman J.D.,Gal-Yam A.
73. Gorbikov E.
74. Higgins D.
75. Janczak J.
76. Kaspi S.
77. Lee C.-U.,Mallia F.
78. Maury A.
79. Monard L.A.G.
80. Moorhouse D.
81. Morgan N.
82. Natusch T.,Ofek E.O.
83. Park B.-G.
84. Pogge R.W.
85. Polishook D.
86. Santallo R.
87. Shporer A.,Spector O.
88. Thornley G.
89. Yee J.C. (The {mu} Collaboration),Bozza V.
90. Browne P.
91. Dominik M.
92. Dreizler S.
93. Finet F.
94. Glitrup M.,Grundah F.
95. Harpsoe K.
96. Hessman F.V.
97. Hinse T.C.
98. Hundertmark M.,Jorgensen U.G.
99. Liebig C.
100. Maier G.
101. Mancini L.
102. Mathiasen M.
103. Rahvar S.,Ricci D.
104. Scarpetta G.
105. Southworth J.
106. Surdej J.
107. Zimmer F.,(The MiNDSTEp Consortium),Allan A.
108. Bramich D.M.
109. Snodgrass C.
110. Steele I.A.
111. Street R.A.(The RoboNet Collaboration)

Published by

CDS

Abstract

We report the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval, one of the longest for any planetary event. The host is an M dwarf, with a mass in the range 0.07M_{sun}_<M_host_<0.49M_{sum}_ at 90% confidence. The planet-star mass ratio q=0.0132+/-0.003 has been measured extremely well, so at the best-estimated host mass, the planet mass is m_p_=2.6 Jupiter masses for the median host mass, M=0.19M_{sun}_.

Keywords

1. multiple-stars
2. solar-system-planets
3. apparent-magnitude

Bibliographic source Bibcode

2011A&A...529A.102B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/529/A102

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/529/A102

Document Object Identifer DOI

doi:10.26093/cds/vizier.35290102

Access

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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/529/A102

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